Probing the Physical Origin of the Balmer Decrement in the Broad-line Region of Nearby Active Galactic Nuclei via Spectral Variability

BibTeX Entry

@article{2025arXiv251107714S,
  author = {{Son}, Suyeon and {Kim}, Minjin and {Ho}, Luis C. and {Li}, Ruancun},
  title = {{Probing the Physical Origin of the Balmer Decrement in the Broad-line Region of Nearby Active Galactic Nuclei via Spectral Variability}},
  journal = {arXiv e-prints},
  keywords = {Astrophysics of Galaxies},
  year = {2025},
  month = nov,
  eid = {arXiv:2511.07714},
  pages = {arXiv:2511.07714},
  archiveprefix = {arXiv},
  eprint = {2511.07714},
  primaryclass = {astro-ph.GA},
  adsurl = {https://ui.adsabs.harvard.edu/abs/2025arXiv251107714S},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System},
  dimensions = {true},
  lrdkeys = {dust, emission lines, non-agn, spectroscopy, variability},
  month_numeric = {11}
}

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